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- W2947763260 abstract "Over 200 lines from H2 and Co, formed in interstellar clouds, contain information on the density and the temperature of the gas. Other lines from metals give the abundance of the elements in the solar neighbourhood. Problems with the interpretation of line intensities are discussed." @default.
- W2947763260 created "2019-06-07" @default.
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- W2947763260 date "1978-01-01" @default.
- W2947763260 modified "2023-09-27" @default.
- W2947763260 title "VI. - NUAGES INTERSTELLAIRES, FORMATION DES ÉTOILES.INTERSTELLAR LINES AND ABUNDANCES FROM THE FAR-U.V." @default.
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